The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model

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	The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model
	Tong H(仝号); Ren-Xin Xu; Song LM(宋黎明)
发表期刊	Research in Astronomy and Astrophysics;2011;第12期;P1371-1376;
通讯作者	仝号
摘要	X-ray dim isolated neutron stars are peculiar pulsar-like objects,characterized by their Planck-like spectrum.In studying their spectral energy distributions,optical/ultraviolet(UV) excess is a long standing problem.Recently Kaplan et al.measured the optical/UV excess for all seven sources,which is understandable in the resonant cyclotron scattering(RCS) model previously addressed.The RCS model calculations show that the RCS process can account for the observed optical/UV excess for most sources.The ?at spectrum of RX J2143.0+0654 may be due to contributions from the bremsstrahlung emission of the electron system in addition to the RCS process.
关键词	Hao China Tong School of Physics and State Key Laboratory of Nuclear Physics and Technology Ren-Xin Xu Li-Ming Song（Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 Peking University Beijing 100871 China）
收录类别	ADS
ADS Bibcode	2011RAA....11.1371T
ADS URL	https://ui.adsabs.harvard.edu/abs/2011RAA....11.1371T
ADS引文	https://ui.adsabs.harvard.edu/abs/2011RAA....11.1371T/citations
引用统计	被引频次：6 [ADS]
文献类型	期刊论文
条目标识符	https://ir.ihep.ac.cn/handle/311005/218075
专题	粒子天体物理中心
推荐引用方式 GB/T 7714	Tong H,Ren-Xin Xu,Song LM. The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model[J]. Research in Astronomy and Astrophysics;2011;第12期;P1371-1376;.
APA	仝号,Ren-Xin Xu,&宋黎明.
MLA	仝号,et al."The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model".Research in Astronomy and Astrophysics;2011;第12期;P1371-1376;